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The Faint Sky Variability Survey – I. Goals and data reduction process
Authors:P. J. Groot  P. M. Vreeswijk  M. E. Huber  M. E. Everett  S. B. Howell  G. Nelemans  J. van Paradijs  E. P. J. van den Heuvel  T. Augusteijn  E. Kuulkers  R. G. M. Rutten   J. Storm
Affiliation:Department of Astrophysics, University of Nijmegen, PO Box 9010, 6500 GL Nijmegen, the Netherlands;Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, 02138 MA, USA;Astronomical Institute 'Anton Pannekoek'/CHEAF, Kruislaan 403, 1098 SJ, Amsterdam, the Netherlands;Astrophysics Group, Planetary Science Institute, 620 N. 6th Ave., Tucson, AZ, USA;Department of Physics and Astronomy, University of Wyoming, PO Box 3905, Laramie, WY 82071, USA;Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA;Physics Department, University of Alabama in Huntsville, Huntsville, USA;Isaac Newton Group of Telescopes, Apartado de Correos 321, 38700 Sta Cruz de La Palma, Canary Islands, Spain;Nordic Optical Telescope, Apartado de Correos 474, 38700 Sta de La Palma, Canary Islands, Spain;ESA-ESTEC, Science Operations and Data Systems Division, SCI-SDG, Keplerlaan 1, 2201 AZ Noordwijk, the Netherlands;Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
Abstract:
Keywords:methods: data analysis    techniques: photometric    surveys    stars: variables: other    Galaxy: stellar content
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